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    "results": [
        {
            "id": 5577,
            "url": "https://svs.gsfc.nasa.gov/5577/",
            "result_type": "Animation",
            "release_date": "2025-11-20T09:00:00-05:00",
            "title": "SDO Sun This Week",
            "description": "This visualization shows SDO AIA-304 imagery from the past 7 days with a color table and image processing applied. Archive folders are provided in the Download menu.",
            "hits": 0
        },
        {
            "id": 4352,
            "url": "https://svs.gsfc.nasa.gov/4352/",
            "result_type": "Visualization",
            "release_date": "2017-08-20T10:00:00-04:00",
            "title": "Incredible Solar Flare, Prominence Eruption and CME Event (SDO/HMI visible light)",
            "description": "These movies present the six hour interval around the event, a one minute per animation frame. || MonsterFilament_HMI_stand.HD1080i.00100_print.jpg (1024x576) [40.8 KB] || MonsterFilament_HMI_stand.HD1080i.00100_searchweb.png (320x180) [21.8 KB] || MonsterFilament_HMI_stand.HD1080i.00100_thm.png (80x40) [2.7 KB] || MonsterFilament_HMI_stand.HD1080i.00100_web.png (320x180) [21.8 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || MonsterFilament_HMI.HD1080i_p30.mp4 (1920x1080) [12.1 MB] || MonsterFilament_HMI.HD1080i_p30.webm (1920x1080) [1.2 MB] || MonsterFilament_HMI.HD1080i_p30.mp4.hwshow [197 bytes] || ",
            "hits": 69
        },
        {
            "id": 12613,
            "url": "https://svs.gsfc.nasa.gov/12613/",
            "result_type": "Produced Video",
            "release_date": "2017-06-02T11:00:00-04:00",
            "title": "SDO 4k Slow-rotation Sun Resource Page",
            "description": "Still Image for page || SDO_Slow_Gallery.jpg (1920x1080) [235.4 KB] || SDO_Slow_Gallery_searchweb.png (320x180) [43.0 KB] || SDO_Slow_Gallery_thm.png (80x40) [3.6 KB] || ",
            "hits": 174
        },
        {
            "id": 12614,
            "url": "https://svs.gsfc.nasa.gov/12614/",
            "result_type": "Produced Video",
            "release_date": "2017-06-02T11:00:00-04:00",
            "title": "SDO Anniversary Series",
            "description": "The sun is always changing and NASA's Solar Dynamics Observatory is always watching. Launched on Feb. 11, 2010, SDO keeps a 24-hour eye on the entire disk of the sun, with a prime view of the graceful dance of solar material coursing through the sun's atmosphere, the corona.Year 1 || ",
            "hits": 71
        },
        {
            "id": 4166,
            "url": "https://svs.gsfc.nasa.gov/4166/",
            "result_type": "Visualization",
            "release_date": "2015-02-11T00:00:00-05:00",
            "title": "March 2014: Erupting Solar Prominence",
            "description": "A solar filament, in the upper left quadrant of the image, erupts from the Sun (about time stamp 2014 March 29 01:54:00 UTC).There is a gap of 40 minutes in the data coverage,  from 03:00 - 03:40 UT. || ",
            "hits": 54
        },
        {
            "id": 4051,
            "url": "https://svs.gsfc.nasa.gov/4051/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "Boiling Solar Prominence from February 2013",
            "description": "A long-lived prominence (see Wikipedia) hovers over the limb of the Sun (about the 4-5 o'clock position) before breaking up. || ",
            "hits": 30
        },
        {
            "id": 4090,
            "url": "https://svs.gsfc.nasa.gov/4090/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "Solar Prominence from SDO: July 1, 2013",
            "description": "A large solar prominence, caught in a tug-of-war between solar gravity pulling it downward and magnetic gradients lifting upward, hovers over the limb of the Sun (left) before eventually launching into space. || ",
            "hits": 48
        },
        {
            "id": 3828,
            "url": "https://svs.gsfc.nasa.gov/3828/",
            "result_type": "Visualization",
            "release_date": "2011-12-07T00:00:00-05:00",
            "title": "Solar Dynamics Observatory - Atmospheric Imaging Assembly",
            "description": "The Sun's activity increases as we enter solar cycle 24. But even several years away from the peak, the Sun in ultraviolet light shows a variety of activity.This visualization consists of eight hours of SDO AIA imagery from the 30.4 nanometer filter (304 Ångstroms). This sequence plays at the full time cadence of the AIA instrument - one image every twelve seconds of real time - and showing thirty images per second on playback. || ",
            "hits": 200
        },
        {
            "id": 3838,
            "url": "https://svs.gsfc.nasa.gov/3838/",
            "result_type": "Visualization",
            "release_date": "2011-07-01T10:00:00-04:00",
            "title": "Incredible Solar Flare, Prominence Eruption and CME Event (304 angstroms)",
            "description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk.Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events.This image sequence is captured at one minute intervals and designed to play synchronously with animations 3839 (171 Ångstroms), 3840 (211 Ångstroms) and 3841 (1700 Ångstroms). || ",
            "hits": 62
        },
        {
            "id": 3839,
            "url": "https://svs.gsfc.nasa.gov/3839/",
            "result_type": "Visualization",
            "release_date": "2011-07-01T10:00:00-04:00",
            "title": "Incredible Solar Flare, Prominence Eruption and CME Event (171 angstroms)",
            "description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk.Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events.This image sequence is captured at one minute intervals and designed to play synchronously with animations 3838 (304 Ångstroms), 3840 (211 Ångstroms) and 3841 (1700 Ångstroms). || ",
            "hits": 80
        },
        {
            "id": 3840,
            "url": "https://svs.gsfc.nasa.gov/3840/",
            "result_type": "Visualization",
            "release_date": "2011-07-01T10:00:00-04:00",
            "title": "Incredible Solar Flare, Prominence Eruption and CME Event (211 angstroms)",
            "description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk.Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events.This image sequence is captured at one minute intervals and designed to play synchronously with animations 3839 (171 Ångstroms), 3838 (304 Ångstroms) and 3841 (1700 Ångstroms). || ",
            "hits": 44
        },
        {
            "id": 3841,
            "url": "https://svs.gsfc.nasa.gov/3841/",
            "result_type": "Visualization",
            "release_date": "2011-07-01T10:00:00-04:00",
            "title": "Incredible Solar Flare, Prominence Eruption and CME Event (1700 angstroms)",
            "description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). At this wavelength, very little of the ejected material is visible. However, it is possible to see locations where some of the material is falling back and striking the solar surface.This image sequence is captured at one minute intervals and designed to play synchronously with animations 3839 (171 Ångstroms), 3840 (211 Ångstroms) and 3838 (304 Ångstroms). || ",
            "hits": 43
        },
        {
            "id": 10610,
            "url": "https://svs.gsfc.nasa.gov/10610/",
            "result_type": "Produced Video",
            "release_date": "2010-04-28T11:00:00-04:00",
            "title": "SDO First Light High Resolution Stills",
            "description": "Stills from the AIA instrument on SDO. They show the March 30, 2010 \"First Light\" prominence eruption captured just after the AIA sensors were activated. All images are from the ultraviolet part of the spectrum, specifically the wavelengths of 304, 211, 193, and 171 Ångstroms. The stills are in multiple resolutions and are available as tiff and jpeg files. || ",
            "hits": 160
        },
        {
            "id": 2960,
            "url": "https://svs.gsfc.nasa.gov/2960/",
            "result_type": "Visualization",
            "release_date": "2004-07-08T12:00:00-04:00",
            "title": "Halloween Solar Storms from SOHO/EIT, 304 Angstroms",
            "description": "This view from SOHO/EIT in the 304 angstrom band, shows a group of active regions rotating back into view. This movie is synchronized to play with animation IDs 2959 and 2961. One obvious difference is that solar flares are not as visible at this wavelength than at the 195 angstrom band. The 304 angstrom filter was not used as frequently as the 195 angstrom filter, so this movie has more jumps in its time coverage. For more information on how X-ray solar flares are classified (B, C, M, X), visit SpaceWeather.com. || ",
            "hits": 30
        }
    ]
}